4.7 Article

Close Binary Companions to APOGEE DR16 Stars: 20,000 Binary-star Systems Across the Color-Magnitude Diagram

期刊

ASTROPHYSICAL JOURNAL
卷 895, 期 1, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4357/ab8acc

关键词

Binary stars; Close binary stars; Radial velocity; Spectroscopy; Astronomy data analysis; Bayesian statistics; Astrostatistics; Surveys

资金

  1. Max-Planck-Institut fur Astronomie
  2. NSF [AST 1616636]
  3. National Science Foundation [AST-1311835, AST-1715662]
  4. FONDECYT [3180210]
  5. Becas Iberoamerica Investigador 2019, Banco Santander Chile
  6. State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) [AYA2017-88254-P]
  7. European Regional Development Fund (FEDER) [AYA2017-88254-P]
  8. NSF Astronomy and Astrophysics Postdoctoral Fellowship [AST-1801940]
  9. U.S. National Science Foundation [PHY 14-30152]
  10. NASA through Hubble Fellowship grant by the Space Telescope Science Institute [51386.01]
  11. NASA [NAS 5-26555]
  12. Alfred P. Sloan Foundation
  13. U.S. Department of Energy Office of Science
  14. Center for High-Performance Computing at the University of Utah
  15. Brazilian Participation Group
  16. Carnegie Institution for Science
  17. Carnegie Mellon University
  18. Chilean Participation Group
  19. French Participation Group
  20. Harvard-Smithsonian Center for Astrophysics
  21. Instituto de Astrofisica de Canarias
  22. Johns Hopkins University
  23. Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
  24. Lawrence Berkeley National Laboratory
  25. Leibniz Institut fur Astrophysik Potsdam (AIP)
  26. Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
  27. Max-Planck-Institut fur Astrophysik (MPA Garching)
  28. Max-PlanckInstitut fur Extraterrestrische Physik (MPE)
  29. National Astronomical Observatories of China
  30. New Mexico State University
  31. New York University
  32. University of Notre Dame
  33. Observatario Nacional/MCTI
  34. Ohio State University
  35. Pennsylvania State University
  36. Shanghai Astronomical Observatory
  37. United Kingdom Participation Group
  38. Universidad Nacional Autonoma de Mexico
  39. University of Arizona
  40. University of Colorado Boulder
  41. University of Oxford
  42. University of Portsmouth
  43. University of Utah
  44. University of Virginia
  45. University of Washington
  46. University of Wisconsin
  47. Vanderbilt University
  48. Yale University

向作者/读者索取更多资源

Many problems in contemporary astrophysics-from understanding the formation of black holes to untangling the chemical evolution of galaxies-rely on knowledge about binary stars. This, in turn, depends on the discovery and characterization of binary companions for large numbers of different kinds of stars in different chemical and dynamical environments. Current stellar spectroscopic surveys observe hundreds of thousands to millions of stars with (typically) few observational epochs, which allows for binary discovery but makes orbital characterization challenging. We use a custom Monte Carlo sampler (The Joker) to perform discovery and characterization of binary systems through radial velocities, in the regime of sparse, noisy, and poorly sampled multi-epoch data. We use it to generate posterior samplings in Keplerian parameters for 232,495 sources released in APOGEE Data Release 16. Our final catalog contains 19,635 high-confidence close-binary (P less than or similar to few years, a less than or similar to few

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